% @(#)adapt_roma.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:17:45 \se SECTION./ROMAFOT \es\co ADAPT/ROMAFOT 08-DEC-1988 RHW \oc\su ADAPT/ROMAFOT int_tab [thres] [fac_int] [fac_sky] [fac_hol] [x_siz,y_siz] derive trial values for fitting a new frame \us\pu Purpose: Use the fit on the template image frame to derive trial values to fit a new frame \up\sy Syntax: ADAPT/ROMAFOT int_tab [thres] [fac_int] [fac_sky] [fac_hol] [x_size,y_size] \ys\pa int_tab = the intermediate table with transformed coordinates by CTRANS/ROMAFOT; no default. \ap\pa thresh = photometric threshold in intensity. Objects with max. intensity under this threshold are flagged and will not be considered in the fit. Nevertheless they are kept in the intermediate table (with flag set to 0) to keep the correspondence with previous registration tables. Default value is 0.0. \ap\pa fac_int = factor to multiply the intensities of the objects in the intermediate table; default 1.0. \ap\pa fac_sky = factor to multiply the intensity of the sky bakground in the intermediate tablep; default 1.0. \ap\pa fac_hol = factor to multiply the radius of holes in the intermediate table; default 1.0. \ap\pa x_size,y_size = dimensions of the new frame to fit; default same size(s) as before. \ap\no Note: None \on\exs Examples: \ex ADAPT/ROMAFOT GCLINT 200 3.2 0.5 1.4 320,520 Flag the objects with central intensity lower than 200 units in the intermediate table GCLINT; for the remainders multiply the fitted central intensity by 3.2, the sky background by 0.5 and, finally, the holes radii by 1.4. Flag the objects which, after the transformation of coordinates, exceed 320 in x and 520 in y. \xe \sxe